New results on the sdB star PG 0014+067

Details New results on the sdB star PG 0014+067 New results on the sdB star PG 0014+067

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jphcs.172a2016b&link_type=abstract

Journal of Physics: Conference Series, Volume 172, Issue 1, pp. 012016 (2009).

Physics

5

Scientific paper

We present here our third generation of sdB star models geared for asteroseismology. As a test of these new models, we return to a thorough analysis of the pulsating sdB PG 0014+067. We also provide a new treatment of the observed data. Many possible working hypotheses for the mode identification have been tested. In an outcome that may seem surprising to some, we found that almost all of them seem to produce very similar seismic models.

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